Microquasars Blowing Macro-bubbles

Details Microquasars Blowing Macro-bubbles Microquasars Blowing Macro-bubbles

Sep 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006head....9.0801h&link_type=abstract

American Astronomical Society, HEAD meeting #9, #8.01; Bulletin of the American Astronomical Society, Vol. 38, p.361

Physics

Scientific paper

Observations of the large scale structure of radio galaxies have been a useful tool to study AGN jet physics for decades. In recent years, it has become clear that X-ray binaries are just as proficient at making jets as supermassive black holes in AGNs, yet, the large scale radio structure surrounding them (far beyond the barely resolvable cores on AU scales) has only been observed in a handful of sources. I will discuss some of the observations in light of theoretical predictions based on our knowledge of radio galaxies. I will argue that radio lobes around X-ray binaries are quite common and provide a powerful tool to study the physics of microquasar jets.

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